Copernicus Crater

Copernicus Crater is a prominent impact crater on the Moon’s surface, approximately 15 kilometers in diameter. It formed around 800 million years ago when a meteoroid struck the lunar surface, creating a circular depression with raised walls and central peaks. The crater’s bright, terraced walls and the central dome are easily visible from Earth with telescopes. Its relatively young age means it has well-defined features. Copernicus is a key reference point for lunar geologists studying impact processes and the Moon’s history. Its striking appearance also makes it one of the most recognizable and photographed lunar craters.